Fig. 7.
Thermodynamic maps of A523. Panel a: temperature map (keV); panel b: metal abundance map (Z⊙); panel c: pseudo-pressure map (arbitrary units); panel d: pseudo-entropy map (arbitrary units). Overlaid to each image are the surface brightness contours obtained by the XMM-Newton image and the positions of the two brightest cluster galaxies are indicated by two black crosses.
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